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20172025
most citedImportance of accurate consideration of the electron inertia in hybrid-kinetic simulations of collisionless plasma turbulence: 1. The 2D limit

9 citations · 9 across the 2 of their papers we have counts for

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5 papers · 1 filter

astro-ph.HE20249 cited

Poynting flux transport channels formed in polar cap regions of neutron star magnetospheres

Jan Benáček, Andrey Timokhin, Patricio A. Muñoz +4

Pair cascades in polar cap regions of neutron stars are considered to be an essential process in various models of coherent radio emissions of pulsars. The cascades produce pair pl…

astro-ph.HE2023

Streaming instability in neutron star magnetospheres: No indication of soliton-like waves

Jan Benáček, Patricio A. Muñoz, Jörg Büchner +1

Coherent radiation of pulsars, magnetars, and fast radio bursts could, in theory, be interpreted as radiation from solitons and soliton-like waves. The solitons are meant to contai…

astro-ph.HE2021

Radio Emission by Soliton Formation in Relativistically Hot Streaming Pulsar Pair Plasmas

Jan Benáček, Patricio A. Muñoz, Alina C. Manthei +1

A number of possible pulsar radio emission mechanisms are based on streaming instabilities in relativistically hot electron-positron pair plasmas. At saturation the unstable waves…

astro-ph.HE2020

Refining pulsar radio emission due to streaming instabilities: Linear theory and PIC simulations in a wide parameter range

Alina C. Manthei, Jan Benáček, Patricio A. Muñoz +1

Several important mechanisms that explain the coherent pulsar radio emission rely on streaming (or beam) instabilities of the relativistic pair plasma in a pulsar magnetosphere. Ho…

astro-ph.HE2020

Ion acceleration in non-relativistic quasi-parallel shocks using fully kinetic simulations

Cedric Schreiner, Patrick Kilian, Felix Spanier +2

The formation of collisionless shock fronts is an ubiquitous phenomenon in space plasma environments. In the solar wind shocks might accompany coronal mass ejections, while even mo…